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Fig. E.1.

Fig. E.1. Refer to the following caption and surrounding text.

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Whisker plot displaying the 68% marginalized confidence intervals for the Hubble constant H0 (km s−1 Mpc−1) and spatial curvature parameter ΩK, derived from both viscous cold dark matter models with a cosmological constant (ΛvCDM and ΛvCDM+ΩK with m = 0 and free m) and the standard ΛCDM model, including its curved extension. The analysis includes different datasets: DESI, CC, BAO, PP and PPS supernova samples. The red vertical dashed line indicates the H0 measurement from R22 (Riess et al. 2022)), while the blue vertical dashed line marks the ΛCDM prediction for a flat universe (ΩK = 0).

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